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Chapter 11: Stars and Galaxies in the Universe

Form 2 Science Bab 11: Stars and Galaxies in the Universe

11.1 Stars and Galaxies in the Universe

The universe consists of billions of galaxies, dust, gas particles, and empty space. A galaxy is a massive system containing millions or billions of stars held together by gravitational attraction, along with gas and interstellar dust.

Types of Galaxies

  • Spiral Galaxies: Disk-shaped with spiral arms spinning outwards from a central core (e.g., Milky Way, Andromeda).
  • Elliptical Galaxies: Oval or egg-shaped with dense central clusters and mostly older stars (e.g., Messier 87, Ursa Major).
  • Irregular Galaxies: Distorted shapes with no definite structure, rich in gas and young stars (e.g., Large Magellanic Cloud, Small Magellanic Cloud).

The Milky Way Galaxy

  • The Milky Way is a medium-sized spiral galaxy.
  • Our Solar System is located on one of the outer spiral arms called the Orion Arm.
  • Contains approximately $200\text{ to }400\text{ billion stars}$.

Life Cycle of a Star (Stellar Evolution)

1. Birth of a Star

  • Stars form inside a nebula (a massive cloud of interstellar gas and cosmic dust, mainly hydrogen and helium).
  • Gravity pulls gas and dust together, increasing pressure and core temperature.
  • When core temperature reaches millions of degrees Celsius, nuclear fusion begins (hydrogen nuclei fuse into helium), forming a protostar which eventually becomes a main sequence star.

2. Death of Stars

When hydrogen fuel in the core is exhausted, the star expands into a Red Giant. The final stage depends on the star's original mass:

  • Medium-sized Star (like our Sun):
    $$\text{Protostar} \rightarrow \text{Main Sequence Star} \rightarrow \text{Red Giant} \rightarrow \text{Planetary Nebula} \rightarrow \text{White Dwarf}$$
  • Large Star:
    $$\text{Protostar} \rightarrow \text{Large Star} \rightarrow \text{Red Supergiant} \rightarrow \text{Supernova Explosion} \rightarrow \text{Neutron Star}$$
  • Supermassive Star:
    $$\text{Protostar} \rightarrow \text{Supermassive Star} \rightarrow \text{Red Supergiant} \rightarrow \text{Supernova Explosion} \rightarrow \text{Black Hole}$$

Characteristics Used to Classify Stars

  • Color & Surface Temperature:
    • Red: Coolest surface temperature ($\approx 2,000\text{ K} - 3,500\text{ K}$).
    • Yellow: Medium surface temperature ($\approx 5,000\text{ K} - 6,000\text{ K}$, e.g., the Sun).
    • Blue: Hottest surface temperature ($\approx 25,000\text{ K} - 50,000\text{ K}$).
  • Brightness (Luminosity): Depends on the star's surface temperature, size, and distance from Earth.
  • Size: Ranging from small white dwarfs to giant stars and supergiants (e.g., Betelgeuse).
  • Distance: Measured in Light Years (ly) — the distance light travels through space in one year ($\approx 9.5 \times 10^{12}\text{ km}$).
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